Search Results - "Matson, Dennis"
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Io: Volcanic thermal sources and global heat flow
Published in Icarus (New York, N.Y. 1962) (01-06-2012)“…► Thermal emission from 240 volcanic features on Io equals 55% of Io’s total heat flow. ► Energy emanating from paterae alone represents 46% of Io’s total heat…”
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Map of Io’s volcanic heat flow
Published in Icarus (New York, N.Y. 1962) (01-12-2015)“…•We have mapped Io’s volcanic heat flow and identified areas of high heat flow.•Volcanic heat flow is far from uniform, suggesting possible mantle…”
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Cryolava flow destabilization of crustal methane clathrate hydrate on Titan
Published in Icarus (New York, N.Y. 1962) (01-08-2016)“…•On Titan, destabilization of crustal MCH by cryolavas can release trapped methane.•This methane contributes to Titan's current atmospheric methane…”
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Io: Heat flow from small volcanic features
Published in Icarus (New York, N.Y. 1962) (01-01-2015)“…•We construct infrared color ratio images of Io from Galileo NIMS data.•Nine new faint thermal sources are identified at high spatial resolution.•All of these…”
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Enceladus: A hypothesis for bringing both heat and chemicals to the surface
Published in Icarus (New York, N.Y. 1962) (01-09-2012)“…► Enceladus’ plumes and thermal anomalies are hydrothermal phenomena. ► Warm subsurface ocean water supplies heat to the surface and to the plumes. ► Dissolved…”
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Enceladus' plume: Compositional evidence for a hot interior
Published in Icarus (New York, N.Y. 1962) (01-04-2007)“…The combined observations of Saturn's moon Enceladus by the Cassini CAPS, INMS and UVIS instruments detected water vapor geysers in which were present…”
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Implications of Rotation, Orbital States, Energy Sources, and Heat Transport for Internal Processes in Icy Satellites
Published in Space science reviews (01-06-2010)“…Internal processes in icy satellites, e.g. the exchange of material from the subsurface to the surface or processes leading to volcanism and resurfacing…”
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An overview of the descent and landing of the Huygens probe on Titan
Published in Nature (08-12-2005)“…Titan, Saturn's largest moon, is the only Solar System planetary body other than Earth with a thick nitrogen atmosphere. The Voyager spacecraft confirmed that…”
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Cassini's geological and compositional view of Tethys
Published in Icarus (New York, N.Y. 1962) (01-08-2016)“…•Tethys exhibits spectral variations unique in the saturnian system.•The formation of Ithaca Chasma is not related to the Odysseus impact event.•Odysseus might…”
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Charting thermal emission variability at Pele, Janus Patera and Kanehekili Fluctus with the Galileo NIMS Io Thermal Emission Database (NITED)
Published in Icarus (New York, N.Y. 1962) (01-09-2012)“…Using the NIMS Io Thermal Emission Database (NITED), a collection of over 1000 measurements of radiant flux from Io’s volcanoes (Davies, A.G. et al. [2012]…”
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Global near-IR maps from Gemini-N and Keck in 2010, with a special focus on Janus Patera and Kanehekili Fluctus
Published in Icarus (New York, N.Y. 1962) (01-11-2014)“…•Global maps of Io’s volcanic activity in 2001 and 2010 differ dramatically.•Thermal emission from Janus Patera is relatively steady from 1996 to 2010.•Thermal…”
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Carbon dioxide on the satellites of Saturn: Results from the Cassini VIMS investigation and revisions to the VIMS wavelength scale
Published in Icarus (New York, N.Y. 1962) (01-04-2010)“…Several of the icy satellites of Saturn show the spectroscopic signature of the asymmetric stretching mode of C–O in carbon dioxide (CO 2) at or near the…”
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Io: Heat flow from dark paterae
Published in Icarus (New York, N.Y. 1962) (01-03-2011)“…► The longitudinal distribution of heat flow due to dark paterae on Io is bimodal. ► The heat flow from dark paterae on Io is larger than from dark volcanic…”
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Io: Loki Patera as a magma sea
Published in Journal Of Geophysical Research (02-09-2006)“…We develop a physical model for Loki Patera as a magma sea. We calculate the total volume of magma moving through the Loki Patera volcanic system every…”
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Atmospheric control of the cooling rate of impact melts and cryolavas on Titan’s surface
Published in Icarus (New York, N.Y. 1962) (01-08-2010)“…As on Earth, Titan’s atmosphere plays a major role in the cooling of heated surfaces. We have assessed the mechanisms by which Titan’s atmosphere, dominantly N…”
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The Cassini/Huygens Mission to the Saturnian System
Published in Space science reviews (01-01-2002)“…The international Cassini/Huygens mission consists of the Cassini Saturn Orbiter spacecraft and the Huygens Titan Probe that is targeted for entry into the…”
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VIMS spectral mapping observations of Titan during the Cassini prime mission
Published in Planetary and space science (01-12-2009)“…This is a data paper designed to facilitate the use of and comparisons to Cassini/visual and infrared mapping spectrometer (VIMS) spectral mapping data of…”
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Post-solidification cooling and the age of Io's lava flows
Published in Icarus (New York, N.Y. 1962) (01-07-2005)“…The modeling of thermal emission from active lava flows must account for the cooling of the lava after solidification. Models of lava cooling applied to data…”
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Hydrated salt minerals on Europa's surface from the Galileo near-infrared mapping spectrometer (NIMS) investigation
Published in Journal of Geophysical Research: Planets (25-05-1999)“…We reported evidence of heavily hydrated salt minerals present over large areas of Europa's surface from analysis of reflectance spectra returned by the…”
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Earth-Based Support for the Titan Saturn System Mission
Published in Earth, moon, and planets (01-09-2009)“…The Titan Saturn System Mission (TSSM) concept is composed of a TSSM orbiter provided by NASA that would carry two Titan in situ elements provided by ESA: the…”
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